CWNU 1854
Summary
CWNU 1854 is a poorly populated, moderately dense object of high C3 quality. It is located at a moderate distance from the Sun, above the mid-plane. It was recently reported in the literature.
This object shares a large percentage of members with a later reported entry.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| He et al. (2023) | 138.724 | -45.3 | 0.451 | -5.558 | 4.069 | – |
| UCC | 138.72 | -45.299 | 0.445 | -5.556 | 4.062 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| He et al. (2023) | A0=1.2, m-M=11.6, logAge=7.3 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| Theia 3317 | 85.7 | 138.72 | -45.3 | 0.44 | -5.56 | 4.06 | – | 0.01 |